Abstract
A new era in fundamental physics began when pulsars were discovered in 1967. Soon it became clear that pulsars were useful tools for a wide variety of physical and astrophysical problems. Further applications became possible with the discovery of the first binary pulsar in 1974 and the discovery of millisecond pulsars in 1982. Ever since pulsars have been used as precise cosmic clocks, taking us beyond the weak-field limit of the solar-system in the study of theories of gravity. Their contribution is crucial as no test can be considered to be complete without probing the strong-field realm of gravitational physics by finding and timing pulsars. This is particularly highlighted by the discovery of the first double pulsar system in 2003. In this review, I will explain some of the most important applications of millisecond pulsar clocks in the study of gravity and fundamental constants.
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References
1. C. M. Will, Living Rev. Relativity 4, 4. [Online article]: cited on 1 Oct 2003, http://www.livingreviews.org/lrr-2001-4 (2001)
2. S.G. Turyshev et al., 35 Years of Testing Relativistic Gravity: Where Do We Go from Here?, Lect. Notes Phys. 648, 311–330 (2004)
3. N. Wex, In: Gyros, Clocks, Interferometers...: Testing Relativistic Gravity in Space, eds C. Lämmerzahl, C. W. F. Everitt, & F. W. Hehl, (Springer, 2001)
4. I. H. Stairs, Living Rev. Relativity 6, 5. [Online article]: cited on 1 Oct 2003, http://www.livingreviews.org/lrr-2003-5 (2003)
5. D. R. Lorimer, Living Rev. Relativity 4, 5. [Online article]: cited on 1 Oct 2003, http://www.livingreviews.org/lrr-2001-5 (2001)
6. S. E. Thorsett & D. Chakrabarty, Ap. J. 512, 288 (1999)
7. J. R. Oppenheimer & G. Volkoff, Phys. Rev. 55, 374 (1939)
8. V. E. Zavlin and G. G. Pavlov, A&A 329, 583 (1998)
9. M. A. McLaughlin, I. H. Stairs, V. M. Kaspi et al., Ap. J. 591, L135 (2003)
10. G. F. Bignami, P. A. Caraveo, A. D. Luca & S. Mereghetti, Nature 423, 725 (2003)
11. T. H. Hankins, J. S. Kern, J. C. Weatherall & J. A. Eilek, Nature 422, 141 (2003)
12. M. Kramer, K. M. Xilouris, A. Jessner, et al., A&A, 322, 846 (1997)
13. A. G. Lyne, R. S. Pritchard & F. G. Smith, MNRAS 265, 1003 (1993)
14. M. Kramer, A. G. Lyne, G. Hobbs, et al., Ap.J. 593, L31 (2003)
15. M. D. Young, R. N. Manchester & S. Johnston, Nature 400, 848 (1999)
16. D. C. Backer, S. R. Kulkarni, C. Heiles, M. M. Davis & W. M.Goss, Nature 300, 615 (1982)
17. M. A. Alpar, A. F. Cheng, M. A. Ruderman & J. Shaham, Nature 300, 728 (1982)
18. V. M. Kaspi, J. H. Taylor & M. Ryba, Ap. J. 428, 713 (1994)
19. E. M. Standish, A&A 114, 297 (1982)
20. I. I. Shapiro, Phys. Rev. Lett. 13, 789 (1964)
21. D. C. Backer & R. W. Hellings, Ann. Rev. Astr. Ap. 24, 537 (1986)
22. E. S. Phinney, Philos. Trans. Roy. Soc. London A341, 39 (1992)
23. http://pulsar.princeton.edu/tempo/
24. http://www.jb.man.ac.uk/research/pulsar/observing/progs/progs.html
25. http://www.mpifr-bonn.mpg.de/div/pulsar/former/olegd/soft.html
26. K. Nordtvedt, Phys. Rev. 170, 1186 (1968)
27. N. Wex, In: Pulsar Astronomy - 2000 and Beyond, IAU Colloquium 177, eds M. Kramer, N. Wex & R. Wielebinski, R., ASP Conf. Series Vol. 202 (PASP, San Francisco 2000), p. 113
28. T. Damour & G. Schäfer, Phys. Rev. Lett. 66, 2549 (1991)
29. C. Lange, F. Camilo, N. Wex et al., MNRAS 326, 274 (2001)
30. C. M. Will, Theory and Experiment in Gravitational Physics, (Cambridge University Press, Cambridge 1993)
31. J. F. Bell, Ap. J. 462, 287 (1996)
32. Bell, J. F. & Damour, T., Class. Quantum Grav., 13, 3121 (1996)
33. C. M. Will, Ap. J. 393, L59 (1992)
34. T. Damour, G. W. Gibbons & J. H. Taylor, Phys. Rev. Lett. 61, 1151 (1988)
35. Z. Arzoumanian, PhD thesis, Princeton University (1995)
36. S. E. Thorsett, Phys. Rev. Lett. 77, 1432 (1996)
37. J. M. Weisberg & J. H. Taylor, In: Radio Pulsars, eds M. Bailes, D.J. Nice & S.E. Thorsett, ASP Conf. Series Vol. 302 (PASP, San Francisco 2003), p. 93
38. T. Damour & G. Esposito-Farèse, Phys. Rev. D53, 5541 (1996)
39. T. Damour & G. Esposito-Farèse, Phys. Rev. D58, 042001 (1998)
40. Esposito-Farèse, G. contribution to 10th Marcel Grossmann meeting, gr-qc/0402007 (2004)
41. I. H. Stairs, S. E. Thorsett, J. H. Taylor & A. Wolszczan, Ap. J. 581, 501 (2002)
42. T. Damour & R. Ruffini, Academie des Sciences Paris Comptes Rendus Ser. Scie. Math. 279, 971 (1974)
43. M. Kramer, Ap. J. 509, 856 (1998)
44. M. Kramer, In: The Ninth Marcel Grossmann Meeting, eds V.G. Gurzadyan, R.T. Jantzen & R. Ruffini (World Scientific, Singapore 2002) p. 219
45. R. N. Manchester, A. G. Lyne, F. Camilo, et al., MNRAS 328, 17 (2001)
46. V. M. Kaspi, A. G. Lyne, R. N. Manchester, et al., Ap. J. 543, 321 (2000)
47. Burgay, M., D’Amico, N., Possenti, et al., Nature, 426, 531 (2003)
48. Lyne, A. G., Burgay, M., Kramer, M., et al., Science, 303, 1153 (2004)
49. Damour, T. & Taylor, J. H., Phys. Rev. D, 45, 1840 (1992)
50. Barker, B. M. & O’Connell, R. F., Phys. Rev. D, 12, 329 (1975)
51. Wex, N., 1995, Class. Quantum Grav., 12, 983 (1995)
52. Damour, T. & Schäfer, G., Nuovo Cim., 101, 127 (1988)
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Kramer, M. (2004). Millisecond Pulsarsas Tools of Fundamental Physics. In: Karshenboim, S.G., Peik, E. (eds) Astrophysics, Clocks and Fundamental Constants. Lecture Notes in Physics, vol 648. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-40991-5_3
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